The Fengyun-3C Radio Occultation Sounder GNOS: a Review of the Mission and Its Early Results and Science Applications
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Atmos. Meas. Tech., 11, 5797–5811, 2018 https://doi.org/10.5194/amt-11-5797-2018 © Author(s) 2018. This work is distributed under the Creative Commons Attribution 4.0 License. The FengYun-3C radio occultation sounder GNOS: a review of the mission and its early results and science applications Yueqiang Sun1,2,3, Weihua Bai1,2,3, Congliang Liu1,2, Yan Liu4, Qifei Du1,2,3, Xianyi Wang1,2, Guanglin Yang5, Mi Liao5, Zhongdong Yang5, Xiaoxin Zhang5, Xiangguang Meng1,2, Danyang Zhao1,2, Junming Xia1,2, Yuerong Cai1,2, and Gottfried Kirchengast6,2,1 1Beijing Key Laboratory of Space Environment Exploration, National Space Science Center, Chinese Academy of Sciences (NSSC/CAS), Beijing, China 2Joint Laboratory on Occultations for Atmosphere and Climate (JLOAC) of NSSC/CAS, Beijing, China, and University of Graz, Graz, Austria 3School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing, China 4National Meteorological Center, Chinese Meteorological Administration, Beijing, China 5National Satellite Meteorological Center, Chinese Meteorological Administration, Beijing, China 6Wegener Center for Climate and Global Change (WEGC) and Institute for Geophysics, Astrophysics, and Meteorology/Institute of Physics, University of Graz, Graz, Austria Correspondence: Congliang Liu ([email protected]) and Weihua Bai ([email protected]) Received: 25 October 2017 – Discussion started: 15 January 2018 Revised: 25 July 2018 – Accepted: 7 August 2018 – Published: 23 October 2018 Abstract. The Global Navigation Satellite System (GNSS) uation and scientific applications establishes confidence that Occultation Sounder (GNOS) is one of the new-generation the GNOS data from the series of FY-3 satellites will provide payloads on board the Chinese FengYun 3 (FY-3) series of important contributions to NWP, GCM, and SWR scientific operational meteorological satellites for sounding the Earth’s communities. neutral atmosphere and ionosphere. FY-3C GNOS, on board the FY-3 series C satellite launched in September 2013, was designed to acquire setting and rising radio occultation (RO) data by using GNSS signals from both the Chinese BeiDou 1 Introduction Navigation Satellite System (BDS) and the US Global Posi- tioning System (GPS). So far, the GNOS measurements and The global navigation satellite system (GNSS) radio oc- atmospheric and ionospheric data products have been vali- cultation (RO) technique (Melbourne et al., 1994; Ware dated and evaluated and then been used for atmosphere- and et al., 1996) for sounding the Earth’s neutral atmosphere ionosphere-related scientific applications. and ionosphere was demonstrated by the proof-of-concept This paper reviews the FY-3C GNOS instrument, RO data Global Positioning System/Meteorology (GPS/MET) mis- processing, data quality evaluation, and preliminary research sion launched in 1995 (Ware et al., 1996; Kursinski et al., applications according to the state-of-the-art status of the FY- 1996; Kuo et al., 1998) as well as the following GNSS RO 3C GNOS mission and related publications. The reviewed missions: the Challenging Mini-satellite Payload (CHAMP; data validation and application results demonstrate that the Wickert et al., 2001, 2002); the Constellation Observing Sys- FY-3C GNOS mission can provide accurate and precise at- tem for Meteorology, Ionosphere and Climate (COSMIC; mospheric and ionospheric GNSS (i.e., GPS and BDS) RO Anthes et al., 2000, 2008; Schreiner et al., 2007), the Gravity profiles for numerical weather prediction (NWP), global cli- Recovery and Climate Experiment (GRACE; Beyerle et al., mate monitoring (GCM), and space weather research (SWR). 2005; Wickert et al., 2005); and the Meteorological Opera- The performance of the FY-3C GNOS product quality eval- tional (MetOp) satellites (Edwards and Pawlak, 2000; Lun- tama et al., 2008). These missions have demonstrated the Published by Copernicus Publications on behalf of the European Geosciences Union. 5798 Y. Sun et al.: The FengYun-3C radio occultation sounder GNOS Figure 1. Timeline of FY-3 series satellites. The FY-3 series satel- lites are the Chinese second-generation polar-orbiting meteoro- logical satellites including AM (morning), PM (afternoon), and EM (evening) orbits, and rainfall types of satellites, which have been/will be launched in three batches (source: Sun et al., 2017). unique properties of the GNSS RO technique – such as high vertical resolution, high accuracy, all-weather capability, and Figure 2. Design (functional block diagram) of GNOS instrument global coverage (Ware et al., 1996; Gorbunov et al., 1996; (source: Du et al., 2016). Rocken et al., 1997; Leroy, 1997; Steiner et al., 1999) – and long-term stability and consistency of different RO mission nals (Wang et al., 2015; Bai et al., 2018). The FY-3C satel- observations (Foelsche et al., 2009, 2011). Therefore, GNSS lite is the first BDS- and GPS-compatible RO sounder with a RO data products (i.e., bending angle, refractivity, tempera- state-of-the-art RO receiver – GNOS (Bai et al., 2012, 2014a; ture, pressure, water vapor, and ionospheric electron density Wang et al., 2015; Du et al., 2016). The following FY-3 se- profiles) have been widely used for numerical weather pre- ries of operational meteorological satellites (Fig. 1) will con- diction (NWP; e.g., Healy and Eyre, 2000; Kuo et al., 2000; tinue to carry GNOS as a major payload. The next one of Healy and Thepaut, 2006; Aparicio and Deblonde, 2008; these satellites is FY-3D, which was launched on 15 Novem- Cucurull and Derber, 2008; Poli et al., 2008; Huang et al., ber 2017 (Liao et al., 2016b; Yang et al., 2017; Sun et al., 2010; Le Marshall et al., 2010; Harnisch et al., 2013), global 2017). climate monitoring (GCM; e.g., Steiner et al., 2001, 2009, The FY-3C GNOS instrument consists of three antennas; 2011, 2013; Schmidt et al., 2005, 2008, 2010; Loescher and three radio frequency units (RFUs); and an electronic unit Kirchengast, 2008; Ho et al., 2009, 2012; Foelsche et al., (EU), which uses high-dynamic, high-sensitivity signal ac- 2011a; Lackner et al., 2011), and space weather research quisition and tracking techniques (Fig. 2). The three RFUs (SWR; Anthes, 2011; Anthes et al., 2008; Arras et al., 2008; are installed close to their corresponding antennas by us- Brahmanandam et al., 2012; Pi et al., 1997; Wickert, 2004; ing sharp cavity filters, to reduce the loss of the cable be- Yue et al., 2015). tween antennas and RFUs. The EU is the major component The development of GNSSs such as China’s BeiDou Nav- of GNOS, which accomplishes the GNSS remote-sensing igation Satellite System (BDS), Russia’s GLObal NAviga- signals’ acquisition and tracking as well as the real-time po- tion Satellite System (GLONASS), and the European Galileo sitioning and carrier phase observations (Wang et al., 2015). system has significantly enhanced the availability and capac- In FY-3C GNOS design, the different features of BDS and ity of the GPS-like satellites, which will make GNSS RO GPS signals have been taken into account, and it can observe even more attractive in the future (Bai et al., 2018). These both the neutral atmosphere and ionosphere by using both new GNSS satellites, together with planned low Earth or- BDS and GPS signals. bit (LEO) missions, will offer many more RO observations As shown in Fig. 2, the FY-3C GNOS instrument involves in the future (Wang et al., 2015; Cai et al., 2017). One of a positioning antenna, a rising occultation antenna, and a set- these LEO missions is China’s GNSS Occultation Sounder ting occultation antenna as part of its physical structure. In (GNOS) on board the FengYun 3 series C (FY-3C) satel- terms of electrical structure, the FY-3C GNOS involves five lite, which was successfully launched on 23 September 2013 antennas because each occultation antenna has an ionosphere (Wang et al., 2013, 2014; Bai et al., 2014b, 2016; Liao et al., occultation antenna and an atmosphere occultation antenna 2015, 2016a, b; Wang et al., 2016; Du et al., 2016). (Bai et al., 2014a, b). The FY-3C GNOS mission was designed and developed by the National Space Science Center, Chinese Academy of Sciences (NSSC/CAS), to sound the Earth’s neutral atmo- sphere and ionosphere by using both the BDS and GPS sig- Atmos. Meas. Tech., 11, 5797–5811, 2018 www.atmos-meas-tech.net/11/5797/2018/ Y. Sun et al.: The FengYun-3C radio occultation sounder GNOS 5799 The positioning antenna is a wide-beam, low-gain antenna the atmospheric delay (Ao et al., 2009) is also calculated on pointing toward zenith, which can track six BDS and eight board the GNOS. The baseband signal is then sampled at a GPS satellites simultaneously. Its measurements are used rate of 100 Hz. For the COSMIC and MetOp missions, the for real-time navigation, positioning, and the LEO satellites’ sampling rate of open-loop tracing is 50 Hz (Sokolovskiy, precise orbit determination (POD) in post-processing. 2001; Sokolovskiy et al., 2007, 2009) and 1000 Hz (von En- The front-view (along the satellite velocity direction) oc- geln et al., 2009), respectively. The performance of the COS- cultation antenna and back-view (satellite anti-velocity di- MIC mission proves that a 50 Hz open-loop sampling rate rection) occultation antenna are used for rising and setting is sufficient to monitor the troposphere (Sokolovskiy, 2001; occultation event tracking, respectively. The FY-3C GNOS Sokolovskiy et al., 2007, 2009), while MetOp uses 1000 Hz can track four BDS and six GPS occultation events simulta- to do a detailed spectrum analysis of the lower troposphere. neously. The atmosphere occultation antennas have a pattern Indeed, the higher the sampling rate, the more detailed the that is wide in azimuth and narrow in elevation. A gain of atmospheric information that can be obtained. Compliant approximately 10 dBi is reached over the coverage range of with the FY-3C satellite downlink capability, FY-3C GNOS about ± 35◦ in azimuth and about ±7:5◦ in elevation (Bai et adopts a 100 Hz open-loop sampling rate, which is proven al., 2014a; Du et al., 2016).